Measurement of the β-p emission of Mg and the breakout from the hot CNO cycle

J.P. Wallace; G. Lotay; P.J. Woods; H.M. David; T. Davinson; A. Alharbi; A. Banu; M. McCleskey; B. Roeder; E. Simmons; A. Spiridon; R. Tribble; L. Trache

doi:10.1063/1.3527240

Measurement of the β-p emission of Mg and the breakout from the hot CNO cycle

J.P. Wallace, G. Lotay, P.J. Woods, H.M. David, T. Davinson, A. Alharbi, A. Banu, M. McCleskey, B. Roeder, E. Simmons, A. Spiridon, R. Tribble, L. Trache

School of Physics and Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Chapter

Abstract

In the astrophysically important reaction Ne(p,γ) Na, the rate is dominated by a single key resonance at 450 keV above the proton-emission threshold in Na. Throughout the last few decades many experiments have been performed aimed at finding the identity of this state. Despite this, the spin-parity of the key resonant state is still up for debate. The present paper describes a new experiment studying the β-delayed proton decay of Mg aimed at solving this issue.

Original language	English
Title of host publication	AIP Conference Proceedings
Pages	429-431
Number of pages	3
Volume	1304
DOIs	https://doi.org/10.1063/1.3527240
Publication status	Published - 1 Jan 2010

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10.1063/1.3527240

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abstract = "In the astrophysically important reaction Ne(p,γ) Na, the rate is dominated by a single key resonance at 450 keV above the proton-emission threshold in Na. Throughout the last few decades many experiments have been performed aimed at finding the identity of this state. Despite this, the spin-parity of the key resonant state is still up for debate. The present paper describes a new experiment studying the β-delayed proton decay of Mg aimed at solving this issue.",

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T1 - Measurement of the β-p emission of Mg and the breakout from the hot CNO cycle

AU - Wallace, J.P.

AU - Lotay, G.

AU - Woods, P.J.

AU - David, H.M.

AU - Davinson, T.

AU - Alharbi, A.

AU - Banu, A.

AU - McCleskey, M.

AU - Roeder, B.

AU - Simmons, E.

AU - Spiridon, A.

AU - Tribble, R.

AU - Trache, L.

PY - 2010/1/1

Y1 - 2010/1/1

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AB - In the astrophysically important reaction Ne(p,γ) Na, the rate is dominated by a single key resonance at 450 keV above the proton-emission threshold in Na. Throughout the last few decades many experiments have been performed aimed at finding the identity of this state. Despite this, the spin-parity of the key resonant state is still up for debate. The present paper describes a new experiment studying the β-delayed proton decay of Mg aimed at solving this issue.

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SN - 9780735408593

VL - 1304

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BT - AIP Conference Proceedings

ER -

Measurement of the β-p emission of Mg and the breakout from the hot CNO cycle

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